1 00:00:06,715 --> 00:00:10,468 This is an image of a galaxy cluster called Abell 2744. 2 00:00:10,635 --> 00:00:14,764 It’s in the constellation Sculptor. It's also been nicknamed Pandora's Cluster. 3 00:00:14,806 --> 00:00:17,892 A bunch of galaxies that are all gravitationally bound together. 4 00:00:19,644 --> 00:00:22,731 So you can see all of these sort of yellow fuzzy galaxies here. 5 00:00:22,731 --> 00:00:24,774 They're all very close to each other. 6 00:00:25,483 --> 00:00:28,528 And all of these are sort of glued together by their mutual gravity. 7 00:00:28,528 --> 00:00:31,322 So, the force of gravity is pulling each galaxy 8 00:00:31,322 --> 00:00:34,784 towards each other galaxy and really sticking them together. 9 00:00:34,784 --> 00:00:38,163 You can kind of think of these like almost cities of galaxies, since there are 10 00:00:38,163 --> 00:00:40,707 so many of them that are living in such close proximity. 11 00:00:43,293 --> 00:00:46,379 This cluster was observed as part of the Hubble Frontier Fields program. 12 00:00:46,546 --> 00:00:51,384 That program aimed to image six galaxy clusters with some of the deepest 13 00:00:51,384 --> 00:00:54,637 Hubble observations of a galaxy cluster that have ever been taken. 14 00:00:56,306 --> 00:00:58,099 These are incredibly deep images. 15 00:00:58,099 --> 00:01:00,560 These are some of the deepest images that we've ever had. 16 00:01:01,061 --> 00:01:03,855 Overall, the goal was to really sort of understand 17 00:01:03,855 --> 00:01:06,941 the deepest physics of how these galaxy clusters are acting 18 00:01:06,941 --> 00:01:08,151 as gravitational lenses, 19 00:01:08,276 --> 00:01:11,279 uncover what the dark matter within these galaxy clusters are doing, 20 00:01:11,279 --> 00:01:14,908 and then get a really great look at the galaxies behind the cluster. 21 00:01:14,908 --> 00:01:18,495 So you can see there are a lot of galaxies in this image that are sort of stretched 22 00:01:18,495 --> 00:01:19,996 into these little blue arcs. 23 00:01:20,246 --> 00:01:22,415 These are all gravitationally lensed galaxies, 24 00:01:22,415 --> 00:01:26,419 so they're being magnified by the gravity of this massive galaxy cluster. 25 00:01:26,419 --> 00:01:30,298 And so that gives us a chance to see sort of smaller, fainter objects that would 26 00:01:30,298 --> 00:01:34,385 otherwise be completely invisible without the aid of this cosmic telescope. 27 00:01:35,970 --> 00:01:36,930 And just like a glass 28 00:01:36,930 --> 00:01:40,558 lens, it collects a lot more light and focuses it back to our telescopes. 29 00:01:40,850 --> 00:01:41,935 So we're able to see much 30 00:01:41,935 --> 00:01:42,852 fainter galaxies than we 31 00:01:42,852 --> 00:01:45,980 otherwise would be able to without the aid of gravitational lensing. 32 00:01:46,231 --> 00:01:49,484 This really gives us a huge boost at being able to see sort of the smallest, 33 00:01:49,484 --> 00:01:51,778 faintest objects in the distant universe. 34 00:01:54,030 --> 00:01:56,032 With this particular galaxy cluster, you're able 35 00:01:56,032 --> 00:01:59,744 to see galaxies that are as far back as about 12 billion years ago. 36 00:02:00,120 --> 00:02:03,873 So we're really pushing back to sort of the early days of the universe. 37 00:02:03,873 --> 00:02:07,585 Overall, the age of the universe now is about 13.8 billion years. 38 00:02:07,585 --> 00:02:11,047 So 12 billion years is sort of the early stages 39 00:02:11,047 --> 00:02:12,757 of when these galaxies would have been forming.